Explicit algebraic expressions for cosmic ray electron number density as a function of position and energy are derived for axisymmetric source distributions in galaxies.
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A review summarizing pitfalls in older CR-MHD models and progress toward more rigorous treatments that connect microphysical CR scales to galactic dynamics.
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The Distribution of Cosmic Ray Electrons in Star-Forming Galaxies
Explicit algebraic expressions for cosmic ray electron number density as a function of position and energy are derived for axisymmetric source distributions in galaxies.
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Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models
A review summarizing pitfalls in older CR-MHD models and progress toward more rigorous treatments that connect microphysical CR scales to galactic dynamics.